L.B. Drissi et al. / Nuclear Physics B 804 [PM] (2008) 307–341 319〈Π ia | stands for the <strong>du</strong>al state associated with the <strong>du</strong>al partition Π + = ˜Π T .Wealsohavethefollowing relationI id =∑|Π ia 〉〈Π ia |, 〈Π ia |Π jb 〉=δ ij δ ab ,(3.30)3d partitionsdefining the resolution of the id<strong>en</strong>tity operator I id .(iv) The number |Π| of unit boxes (cubes) of the 3d partition is defined as|Π|= ∑ i,aΠ i,a .(3.31)(v) The boundary (∂Π) of the 3d partition Π is giv<strong>en</strong> by the 2d profile of the correspondingg<strong>en</strong>eralized Young diagram. As this property is important for the pres<strong>en</strong>t study, let give somedetails.Giv<strong>en</strong> a 3d partition Π,theboundary term on the plane x i = N i is a Young diagram (2d partition).On the planes x 1 = N 1 , x 2 = N 2 and x 3 = N 3 , the boundary of Π is composed of by three 2dpartitions λ, μ and ν. So we th<strong>en</strong> have:∂Π = (λ,μ,ν).(3.32)Particular boundaries are giv<strong>en</strong> by the case where a 2d partition is located at infinity; that is thereis no boundary. We distinguish the following situations:∂Π = (∅,μ,ν),∂Π = (∅, ∅,ν),∂Π = (∅, ∅, ∅),where ∅ stands for the vacuum.(3.33)(vi) A conv<strong>en</strong>i<strong>en</strong>t way to deal with 3d partitions is to slice them as a sequ<strong>en</strong>ce of 2d partitionswith interlacing relations. We mainly distinguish two kinds of sequ<strong>en</strong>ces of 2d partitions:perp<strong>en</strong>dicular and diagonal. We will not need this property here; but for details on this mattersee for instance [30] and refer<strong>en</strong>ces therein.β) 4d partitions The 4d partitions P are ext<strong>en</strong>sions of the 3d partitions Π considered above.They can be imagined as 4d g<strong>en</strong>eralized Young diagrams described by the typical integral rank3-t<strong>en</strong>sor,P iaα ∈ Z + , with P iaα P (i+j)(a+b)(α+β) ,(3.34)with 1 i N 1 ,1 a N 2 and 1 α N 3 .Several properties of 2d and 3d partitions ext<strong>en</strong>d to the 4d case; there are also specific propertiesin particular those concerning their slicing into lower-dim<strong>en</strong>sional ones. Below we describesome particular properties of 4d partitions by considering special repres<strong>en</strong>tations.Sub-classes of 4d partitions are giv<strong>en</strong> by:(i) the pro<strong>du</strong>ct of a 2d and a 3d partitions μ and Π likeP = μ ⊗ Π, (P iaα ) = (μ i Π aα ),(3.35)
320 L.B. Drissi et al. / Nuclear Physics B 804 [PM] (2008) 307–341with i = 1,...,N 1 ; a = 1,...,N 2 and α = 1,...,N 3 ,(ii) the pro<strong>du</strong>ct of three kinds of 2d partitionsP = λ ⊗ μ ⊗ ν, (P iaα ) = (λ i μ a ν α ).(3.36)The boundary ∂P of a g<strong>en</strong>eric 4d partition P can be defined in two ways. First in terms of 3dpartitions as follows∂P = (Λ,Π,Σ,Υ).We also have the following particular boundary conditionscase I:case II:case III:case IV:∂P = (∅,Π,Σ,Υ),∂P = (∅, ∅,Σ,Υ),∂P = (∅, ∅, ∅,Υ),∂P = (∅, ∅, ∅, ∅),where ∅ stands for the “3d vacuum” (no boundary condition).Second by using 2d partitions to define boundary of P like(3.37)(3.38)∂P = ( [a, b, c]; [d, e, f]; [g, h, i]; [j, k, l] ) ,where [a, b, c],...and [j, k, l] stand for the boundaries of the 3d partitions Λ,...and Υ .Notice that the second repres<strong>en</strong>tation is more richer since along with the configuration(3.39)∅ =[∅, ∅, ∅],we have moreover the two following extra configurations(3.40)[∅, b, c],[∅, ∅, c].For the case I of Eq. (3.38) correspond th<strong>en</strong> the three following boundary configurations⎧⎪⎨case i: ([∅, b, c]; [d, e, f]; [g, h, i]; [j, k, l])∂P = case ii: ([∅, ∅, c]; [d, e, f]; [g, h, i]; [j, k, l]),⎪⎩case iii: ([∅, ∅, ∅]; [d, e, f]; [g, h, i]; [j, k, l]) ∣(3.41)(3.42)where the last one (case iii) is the case I described by the first relation of Eq. (3.38).This property indicates that one disposes of differ<strong>en</strong>t ways to deal with 4d partitions eitherthe simplest one using 3d-partitions or the more refined on involving 2d partitions. Below weconsider both repres<strong>en</strong>tations.Notice moreover that giv<strong>en</strong> a 4d partition P, we can associate to it various kinds of transposepartitions. Using the particular realization Eq. (3.36), the corresponding transposes read asλ T ⊗ μ ⊗ ν, λ ⊗ μ T ⊗ ν, λ ⊗ μ ⊗ ν T ,λ T ⊗ μ T ⊗ ν, λ ⊗ μ T ⊗ ν T , λ T ⊗ μ ⊗ ν T , λ T ⊗ μ T ⊗ ν T ,(3.43)where λ T stands for the usual transpose of the Young diagram λ.The exact mathematical definitions and the full properties of 4d partitions are not our immediateobjective here; they need by themselves a separate study. Here above we have giv<strong>en</strong> just th<strong>en</strong>eeded properties to set up the structure of the 4-vertex formalism and its restricted non-planar3-vertex method.
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TABLE DES MATIÈRES3.3 Invariants t
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TABLE DES MATIÈRES8.2 Fonctions de
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Avant ProposCe travail à été eff
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10Lab/UFR PHE
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Contributions à l’Etude du Verte
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Contributions à l’Etude du Verte
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du vertex U 3r α = |z 1 | 2 − |z
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H. Jehjouhprojectif complexe -PT d
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Cela a fait apparaître d’autres
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4.2 Fonction de partition perpendic
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4.3 Version raffinée de la fonctio
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4.5 Invariants topologiques dans le
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(Γ + (z) = exp −i ∑ )1n z−n
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Fonctions de Schur et MacMahontopol
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Fonctions de Schur et MacMahonayant
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Bibliographie[1] J. Polchinski, Str
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BIBLIOGRAPHIE[27] A.A. Belavin, A.
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BIBLIOGRAPHIE[57] A. Braverman and
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BIBLIOGRAPHIE[87] Yukiko Konishi, I
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BIBLIOGRAPHIE[119] D. A. Cox, The H
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BIBLIOGRAPHIE[150] C. Weiss and M.
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BIBLIOGRAPHIE[180] H. Awata and H.
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UNIVERSITÉ MOHAMMED V - AGDALFACUL